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Houston Geological Society Bulletin

Abstract


Houston Geological Society Bulletin, Volume 34, No. 9, May 1992. Pages 17-17.

Abstract: Hydrocarbon Geology of Southern Offshore Malta

By

William F. Bishop and Godwin Debono

The study area is 4.4 km. south of Malta, and encompasses 13,000 sq. km. Studies of over 4700 km. of new and reprocessed geophysical data were conducted in 1989-90. These data, supported by stratigraphic projections from the Ragusa basin of Sicily and the Pelagian shelf off Tunisia and Libya, indicate an entirely different facies from the continuous carbonate sequence of the Malta platform encountered by wells drilled to date.

Area 4 is part of the Pelagian block, a stable projection of the African continental margin, bounded on the east by the Ionian abyssal basin; on the west by the N-S axis of Tunisia; on the north by the Calabrian thrust zone; and on the south by the Djeffara flexure. Geologic structures in the study area range from a broad featureless rise to complex horst and graben systems. The latter are mostly of Miocene- Pliocene age, but one graben is believed to represent an early Mesozoic rift associated with breakup of the Pangaea continent.

Carbonates, mostly shallow-water, of Triassic and Jurassic ages were penetrated north of the study area, but source rocks similar to those of the Ragusa basin are postulated in the Mesozoic rift. Several wells encountered Upper Jurassic-Cretaceous carbonates, mostly restricted shelf dolomite, but pelagic limestone beneath a tongue of dolomite at Aqualta-1 indicates this well to be near the southern edge of the Malta platform. During Cretaceous time most of the study area was transitional between platform and basin, and deeper-water strata, which are proven or potential source rocks and seals in Tunisia, should be present. Shelf-edge carbonates will provide good reservoirs, and rudistid reefs probably developed on bathymetric highs. A low-velocity interval at the base of Tertiary section, which wedges out in the southwestern portion of the study area, is expected to contain nummulitid bank facies in contact with deeper-water limestone and marl, which are the source of oil in the giant fields off Tunisia and Libya.

Based on the geothermal gradient at Aqualta-1, the top of the oil window may be about 3000m., and since the entire Jurassic section is below 3500m., it should be capable of peak oil generation. Cretaceous source rocks reached maturity in the southeastern part of the study area during Miocene time and elsewhere since the Pliocene. Restored seismic sections indicate onset of generation at the end of Cretaceous time, when many structures already were positive, others having developed since then. A variety of potential traps, including fault-block, horst, faulted and simple domes and anticlines, are present, together with the very impressive Lower Tertiary wedge-out. Thus, Area 4 is highly prospective and has potential for major hydrocarbon reserves.

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